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The thermal state of molecular clouds in the Galactic center: evidence for non-photon-driven heating
Journal article   Open access  Peer reviewed

The thermal state of molecular clouds in the Galactic center: evidence for non-photon-driven heating

Y. Ao, C. Henkel, K. M. Menten, M. A. Requena-Torres, T. Stanke, R. Mauersberger, S. Aalto, S. Mühle and J. Mangum
Proceedings of the International Astronomical Union, Vol.9(S303), pp.89-91
01/10/2013

Abstract

Contributed Papers
We have used the Atacama Pathfinder Experiment (APEX) 12 m telescope at 218 GHz to observe molecular clouds simultaneously in the JKaKc = 303→202, 322→221, and 321→220 transitions of para-H2CO to determine kinetic temperatures of the dense gas in the central molecular zone of the Galaxy. Gas kinetic temperatures for individual molecular clouds range from 55 to 125 K or even higher. The molecular clouds at high temperatures may be heated by turbulent dissipation and/or cosmic-rays.
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https://doi.org/10.1017/S1743921314000234View
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